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Titan's gravity field and interior structure after Cassini
DOI: 10.1016/j.icarus.2019.03.003 Bibcode: 2019Icar..326..123D

Iess, L.; Durante, Daniele; Hemingway, D. J. +2 more

Since its arrival at Saturn in 2004, Cassini performed nine flybys devoted to the determination of Titan's gravity field and its tidal variations. Here we present an updated gravity solution based on the final data set collected during the gravity-dedicated passes, before Cassini's plunge into Saturn's atmosphere. The data set includes an addition…

2019 Icarus
Cassini 77
Isotopic ratios of Saturn's rings and satellites: Implications for the origin of water and Phoebe
DOI: 10.1016/j.icarus.2018.11.029 Bibcode: 2019Icar..321..791C

Clark, Roger N.; Brown, Robert H.; Cruikshank, Dale P. +1 more

Isotopic ratios have long been used to learn about physical processes acting over a wide range of geological environments, and in constraining the origin and/or evolution of planetary bodies. We report the spectroscopic detection of deuterium in Saturn's rings and satellites, and use these measurements to determine the (D/H) ratios in their near-s…

2019 Icarus
Cassini 37
Observations of the chemical and thermal response of 'ring rain' on Saturn's ionosphere
DOI: 10.1016/j.icarus.2018.10.027 Bibcode: 2019Icar..322..251O

Baines, Kevin H.; O'Donoghue, James; Moore, Luke +4 more

In this study we performed a new analysis of ground-based observations that were taken on 17 April 2011 using the 10-metre Keck telescope on Mauna Kea, Hawaii. Emissions from H3+, a major ion in Saturn's ionosphere, were previously analyzed from these observations, indicating that peaks in emission at specific latitudes were …

2019 Icarus
Cassini 28
Kronoseismology III: Waves in Saturn's inner C ring
DOI: 10.1016/j.icarus.2018.10.013 Bibcode: 2019Icar..319..599F

Nicholson, Philip D.; French, Richard G.; McGhee-French, Colleen A. +1 more

We investigate waves driven in Saturn's rings by planetary normal modes, concentrating on the previously unexplored inner C ring. In this region, the known waves all have exceptionally short wavelengths, which has proven problematic for previous studies that depended on the accurate estimate of wave phases for wave identification. However, detaile…

2019 Icarus
Cassini 26
Cassini-VIMS observations of Saturn's main rings: II. A spectrophotometric study by means of Monte Carlo ray-tracing and Hapke's theory
DOI: 10.1016/j.icarus.2018.07.010 Bibcode: 2019Icar..317..242C

Clark, R. N.; Nicholson, P. D.; D'Aversa, E. +9 more

This work is the second in a series of manuscripts devoted to the investigation of the spectrophotometric properties of Saturn's rings from Cassini-VIMS (Visible and Infrared Mapping Spectrometer) observations. The dataset used for this analysis is represented by ten radial spectrograms of the rings which have been derived in Filacchione et al. (2…

2019 Icarus
Cassini 25
Jupiter's auroral-related stratospheric heating and chemistry III: Abundances of C2H4, CH3C2H, C4H2 and C6H6 from Voyager-IRIS and Cassini-CIRS
DOI: 10.1016/j.icarus.2019.03.012 Bibcode: 2019Icar..328..176S

Fletcher, L. N.; Irwin, P. G. J.; Orton, G. S. +4 more

We present an analysis of Voyager-1-IRIS and Cassini-CIRS spectra of Jupiter's high latitudes acquired during the spacecrafts' respective flybys in November 1979 and January 2001. We performed a forward-model analysis in order to derive the abundances of ethylene (C2H4), methylacetylene (CH3C2H), diacety…

2019 Icarus
Cassini 22
The Cassini VIMS archive of Titan: From browse products to global infrared color maps
DOI: 10.1016/j.icarus.2018.09.017 Bibcode: 2019Icar..319..121L

Le Mouélic, S.; Cornet, T.; Rodriguez, S. +11 more

We have analyzed the complete Visual and Infrared Mapping Spectrometer (VIMS) data archive of Titan. Our objective is to build global surface cartographic products, by combining all the data gathered during the 127 targeted flybys of Titan into synthetic global maps interpolated on a grid at 32 pixels per degree (∼1.4 km/pixel at the equator), in …

2019 Icarus
Cassini 21
Compositional variations of Titan's impact craters indicates active surface erosion
DOI: 10.1016/j.icarus.2018.12.007 Bibcode: 2019Icar..321..508W

Janssen, M. A.; Cassini Radar Team; Werynski, A. +2 more

Titan, the only moon in the solar system with a considerable atmosphere, is host to a variety of exogenic processes that shape its surface. These processes form features that are quite similar to features on Earth, including sand dunes, rivers, and lakes. The combination of a thick atmosphere and active surface processes also leads to a scarcity o…

2019 Icarus
Cassini 18
Spatial and seasonal variations in C3Hx hydrocarbon abundance in Titan's stratosphere from Cassini CIRS observations
DOI: 10.1016/j.icarus.2018.08.027 Bibcode: 2019Icar..317..454L

Lombardo, Nicholas A.; Nixon, Conor A.; Achterberg, Richard K. +4 more

Of the C3Hx hydrocarbons, propane (C3H8) and propyne (methylacetylene, CH3C2H) were first detected in Titan's atmosphere during the Voyager 1 flyby in 1980. Propene (propylene, C3H6) was first detected in 2013 with data from the Composite InfraRed Spectrometer …

2019 Icarus
Cassini 18
Interior properties of the inner Saturnian moons from space astrometry data
DOI: 10.1016/j.icarus.2019.01.026 Bibcode: 2019Icar..326...48L

Lainey, V.; Noyelles, B.; Rambaux, N. +3 more

During the thirteen years in orbit around Saturn before its final plunge, the Cassini spacecraft provided more than ten thousand astrometric measurements. Such large amounts of accurate data enable the search for extremely faint signals in the orbitalmotion of the saturnian moons. Among these, the detection of the dynamical feedback of the rotatio…

2019 Icarus
Cassini eHST 14